The response of a neutron star to the presence of the tidal field, is described by a dimensionless tidal parameter, the tidal Love number \(k_2\) . This parameter depends on the neutron star structure; hence its mass and EoS. The tidal Love number \(k_2\)  is the coefficient of proportionality between the induced quadrupole moment \(Q_{ij}\)  and the applied tidal field \(E_{ij}\)  [1]}, [2]}, given below
\(Q_{ij}=-\frac{2}{3}k_2\frac{R^5}{G}E_{ij}\equiv - \lambda E_{ij},\) 
